Facility acknowledgment for publications
All users are asked to submit information about their resulting publications to the FRIB Manager for User Relations (useroffice@frib.msu.edu). In the future, publication information will be entered on the FRIB Scientific User Portal.
To the extent possible, an acknowledgment of Federal support must appear in the publication of any material, whether copyrighted or not, based on or developed using FRIB resources, as follows:
- Acknowledgment: "This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics and used resources of the Facility for Rare Isotope Beams (FRIB) Operations, which is a DOE Office of Science User Facility under Award Number DE-SC0023633.”
Users must submit their publication information to the DOE Energy Link (E-Link) System.
Proton inelastic scattering in ${}^{68,70,72}Ni$ isotopes
doi: 10.1393/ncc/i2021-21077-6
Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
doi: 10.3847/1538-4357/abfb65
Competition between allowed and first-forbidden β decays of 208At and expansion of the 208Po level scheme
doi: 10.1103/PhysRevC.103.054327
Investigation of the isoscalar response of 24Mg to 6Li scattering
doi: 10.1103/PhysRevC.104.014607
Certification testing of production superconducting quarter-wave and half-wave resonators for FRIB
doi: 10.1016/j.nima.2021.165675
Nuclear Data Sheets for A=123
doi: 10.1016/j.nds.2021.05.001
Improved naive Bayesian probability classifier in predictions of nuclear mass
doi: 10.1103/PhysRevC.104.014315
X-ray burst ignition location on the surface of accreting X-ray pulsars: can bursts preferentially ignite at the hotspot?
doi: 10.1093/mnras/stab1659
Chiral Effective Field Theory and the High-Density Nuclear Equation of State
doi: 10.1146/annurev-nucl-102419-041903
Rodeo Algorithm for Quantum Computing
doi: 10.1103/PhysRevLett.127.040505
Charge balance functions for heavy-ion collisions at energies available at the CERN Large Hadron Collider
doi: 10.1103/PhysRevC.104.014906
Self-consistent 3D Supernova Models From −7 Minutes to +7 s: A 1-bethe Explosion of a ~19 M⊙ Progenitor
doi: 10.3847/1538-4357/abf82e
